‘Super earths’ outside our solar system that are rich in hydrogen or helium may be even MORE habitable than our own planet, study suggests

• Liquid water could exist for billions of years on planets very different from Earth
• They likely ‘bare little resemblance’ to Earth and host organisms at high pressure
• They have atmospheres rich hydrogen or helium, like Earth in its early history

‘Super earths’ outside our solar system that are rich in hydrogen or helium may be even more habitable than our own planet, a new study suggests.

Researchers say rocky exoplanets with atmospheres dominated by hydrogen and helium have surfaces warm enough to host liquid water.

The presence of liquid water is ‘favourable for life’, so these planets could provide habitable conditions and exotic habitats for maybe even 8 billion years. 

Researchers say rocky exoplanets – planets outside our Solar System – with primordial atmospheres dominated by hydrogen and helium have surfaces warm enough to host liquid water

The new study has been led by researchers at the University of Zurich, Switzerland and published today in the journal Nature Astronomy.

EXOPLANETS AND SUPER EARTHS 

An exoplanet is any planet beyond our solar system. Most orbit other stars, but free-floating exoplanets, called rogue planets, orbit the galactic center and are untethered to any star.

Exoplanets found so far include small, rocky worlds like Earth, gas giants many times larger than Jupiter, and ‘hot Jupiters’ in scorchingly close orbits around their stars. 

Meanwhile, a super earth is an exoplanet with a mass higher than that of our home planet. 

Super earths can be made of gas, rock or a combination of both. 

 

They say these planets likely ‘bare very little resemblance to our home planet’ and may host organisms at very high pressures. 

‘Life on the type of planet described in this work would live under considerably different conditions than most life on Earth,’ the authors say. 

‘The surface pressures in our results are on the order of 100–1,000bar, the pressure range of oceanic floors and trenches.

‘There is no theoretical pressure limit on life, and some of the most extreme examples in Earth’s biosphere thrive at around 500bar.’ 

Billions of years ago, the early universe contained only hydrogen and helium, gases, which were readily available in the planet-forming materials around young stars, such as our sun.

Therefore, all planets built up atmospheres that were dominated by these two elements, including Earth. 

‘When the planet first formed from out of cosmic of gas and dust, it collected an atmosphere consisting mostly of hydrogen and helium – a so-called primordial atmosphere,’ said study author Ravit Helled at the University of Zurich. 

Over the course of their development, however, rocky planets including Earth lost this primordial atmosphere in favour of heavier elements, such as oxygen and nitrogen.

However, other, more massive planets can collect much larger primordial atmospheres, which they can keep indefinitely in some cases.

‘Such massive primordial atmospheres can also induce a greenhouse effect – much like Earth’s atmosphere today,’ said Helled.

‘We therefore wanted to find out if these atmospheres can help to create the necessary conditions for liquid water.’ 

For the study, the team modelled nearly 5,000 exoplanets, some bounded to their star and some free floating, and simulated their development over billions of years. 

Researchers accounted not only for properties of the planets’ atmospheres but also the intensity of the radiation of their respective stars as well as the planets’ internal heat radiating outwards. 

While on Earth, this geothermal heat plays only a minor role for the conditions on the surface, it can contribute more significantly on planets with massive primordial atmospheres.

An exoplanet is any planet beyond our solar system. Most orbit other stars, but free-floating exoplanets, called rogue planets, orbit the galactic center and are untethered to any star (file photo) 

Findings suggest that depending on the mass of the planet and how far away it is from its star, these planets could keep a temperate surface environment for as long as 8 billion years, provided the atmosphere is thick enough – between 100 to 1,000 times thicker than the Earth’s. 

‘What we found is that in many cases, primordial atmospheres were lost due to intense radiation from stars, especially on planets that are close to their star,’ said Marit Mol Lous, PhD student and lead author. 

‘But in the cases where the atmospheres remain, the right conditions for liquid water can occur.’

‘In cases where sufficient geothermal heat reaches the surface, radiation from a star like the Sun is not even necessary so that conditions prevail at the surface that allow the existence of liquid water.’ 

‘Perhaps most importantly, our results show that these conditions can persist for very long periods of time – up to tens of billions of years.’ 

The researchers say instruments such as the James Webb Space Telescope, currently in space, and the Extremely Large Telescope, cuyrrently in development, should reveal more about biomarkers in exoplanets’ atmospheres. 

NASA CONFIRMS THERE ARE MORE THAN 5,000 PLANETS BEYOND OUR SOLAR SYSTEM 

NASA has confirmed that there are more than 5,000 known planets outside our solar system, known as exoplanets. 

The US space agency has added another 65 exoplanets to the online NASA Exoplanet Archive, bringing the grand total to 5,009, as of April 1, 2022.

This number was at 5,005 on March 22, showing that four planets had been added to the total in just 10 days.

As of June 8, there are 5,044 exoplanets, the database shows. 

Exoplanets found so far include small, rocky worlds like Earth, gas giants many times larger than Jupiter, and ‘hot Jupiters’ in scorchingly close orbits around their stars. 

The more than 5,000 exoplanets confirmed in our galaxy so far include a variety of types – among them a mysterious variety known as ‘super-Earths’ because they are larger than our world and possibly rocky

However, NASA stresses that only ‘a tiny fraction’ of all the planets in the Milky Way galaxy alone have been found.   

The majority of exoplanets are gaseous, like Jupiter or Neptune, rather than terrestrial, according to NASA’s online database.     

Most exoplanets are found by measuring the dimming of a star that happens to have a planet pass in front of it, called the transit method. 

Another way to detect exoplanets, called the Doppler method, measures the ‘wobbling’ of stars due to the gravitational pull of orbiting planets.  

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